Hawking radiation in GHS and non-extremal D1-D5 blackhole via covariant anomalies

Details Hawking radiation in GHS and non-extremal D1-D5 blackhole via covariant anomalies Hawking radiation in GHS and non-extremal D1-D5 blackhole via covariant anomalies

2007-10-04

arxiv.org/abs/0710.0974v1

Phys.Rev.D77:024038,2008

Physics

High Energy Physics

High Energy Physics - Theory

8 pages latex file

Scientific paper

10.1103/PhysRevD.77.024038

We apply the method of Banerjee and Kulkarni (arXiv:0707.2449, [hep-th]) to
provide a derivation of Hawking radiation from the GHS (stringy) blackhole
which falls in the class of the most general spherically symmetric blackholes
($\sqrt{-g}\neq 1$) and also the non-extremal $D1-D5$ blackhole using only
covariant gravitational anomalies.

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